As I see it a major theme emerging for 2008 is different QG approaches CONVERGING.
Like different climbing teams making their ways up different sides of the same mountain.
A good reason to have a map in the first place is to be able to anticipate convergences.
It looks like in 2007, with the new Marseille spinfoam, the spinfoam approach made solid contact with canonical LQG-----the immirzi showed up, and discrete geometric spectra, and spinfoam seemed to work as a time-evolution joining an initial final spinnetwork state of geometry.
So it's fair of Dittrich to lump all these approaches together in one:
LQG-spinfoam-LQC, the last being application to cosmology and lately also to study what goes on inside the black hole horizon and what replaces the singularity.
The way Dittrich laid it out there were just two main areas Triangulations and Loop.
(somehow other things like Causal Sets and Asymptotic Safety did not get emphasized)
So I want to be alert to anything that looks like a BRIDGE between Triangulations and Loop.
Some PF posters f-h and francesca and maybe also Alejandro Satz have clued us to watch out for Eugenio Bianchi. Here is a December 2007 talk of his at Utrecht:
http://www1.phys.uu.nl/wwwitf/Seminars/Quistabstracts.htm#Bianchi
E. Bianchi (Scuola Normale Superiore, Pisa) - 13 December 2007
Simplicial Geometry from Loop Quantum Gravity
"The relation between Loop Quantum Gravity and simplicial geometry has been pointed out many times in the literature, both at the kinematical and at the dynamical level. In the first part of this talk I will present some new results about the curvature operator in Loop Quantum Gravity and show that appropriate superpositions of spin-network states have curvature with support on one-dimensional hinges, reproducing a three-dimensional simplicial geometry. The second part of the talk is devoted to the dynamics, introduced in terms of a spinfoam model. I will present an analysis of 2- and 3-spin correlation functions on a semiclassical state peaked on flat space and show that they can be reproduced computing in perturbative-Regge-calculus correlations of two and three area-fluctuations around flat space. This analysis is meant to be an intermediate step towards understanding if Loop Quantum Gravity admits a regime which can be described in terms of perturbative (continuum) quantum gravity on flat space."
This talk was at a seminar series that Renate Loll runs at the Utrecht ITF.
Around the same time (mid December) Bianchi and Modesto got a paper about this accepted for publication in Nuclear Physics B, here is the preprint
http://arxiv.org/abs/0709.2051
The perturbative Regge-calculus regime of Loop Quantum Gravity
Eugenio Bianchi, Leonardo Modesto
43 pages, accepted by Nucl.Phys.B
(Submitted on 13 Sep 2007, revised 11 Dec 2007)
"The relation between Loop Quantum Gravity and Regge calculus has been pointed out many times in the literature. In particular the large spin asymptotics of the Barrett-Crane vertex amplitude is known to be related to the Regge action. In this paper we study a semiclassical regime of Loop Quantum Gravity and show that it admits an effective description in terms of perturbative area-Regge-calculus. The regime of interest is identified by a class of states given by superpositions of four-valent spin networks, peaked on large spins.
As a probe of the dynamics in this regime, we compute explicitly two- and three-area correlation functions at the vertex amplitude level. We find that they match with the ones computed perturbatively in area-Regge-calculus with a single 4-simplex, once a specific perturbative action and measure have been chosen in the Regge-calculus path integral. Correlations of other geometric operators and the existence of this regime for other models for the dynamics are briefly discussed."
I am picturing Loll Triangulations and Rovelli Loop as two amoebas beginning to grope for each other and the question is Who Eats Whom?
I think I see about 20 times more researchers and talent on the Loop side. When those two bodies of research get together what does the result look like? More like T'ation or more like Loop?
Maybe it doesn't matter. I think it looks more like Triangulation in spite of the 20-fold imbalance.
I'm impressed that in their model they have found quantum spacetime foam---not putting it in by hand. A foamy, fractally geometry has been expected for 50 years. It came naturally up for them
I'm impressed by the extreme simplicity. They just continue the Quantum Field Theory program inventing nothing and changing as little as possible. Perturbative has been shown not to work, so they go nonperturbative (as QCD did and moved to a lattice) and to avoid the lattice dependence on a fixed background they moved to a free triangulation.
The bare minimum of concepts and of changes to established method.
All path integral method must use some regularization. Theirs is as similar to Feynman's as i can imagine. it is called
piecewise linear. Instead of line segments for a particle path, triangulations describing a path thru piecewise linear geometries. I am impressed by the mathematical naturalness and conservatism.
I'm impressed that they are running computer sims using the full model. Small universes pop into existence, swell up, shrink down, and disappear (back into the minimal geometry state). In Loop cosmology they run simulations but this is not done using the full LQG-spinfoam. It is done with a symmetry-reduced model with only a few degrees of freedom. Triangulations is the only approach where they do full-model simulations of universes.